State-of-art Simulations and Observations for Star Formation

Abstract

In recent year, the formation and formation of galaxies is a hot spot in astrophysics which has been widely investigated and discussed. On the basis of the theory of formation and formation of large-scale structures in modern cosmology, this study intends to systematically investigate and analyze the physical characteristics of galaxies in different stages, such as morphological structure, star family structure, gas accretion, stellar formation, black hole growth, chemical elements, stellar and gas movements, and their physical relationships with large-scale structures. According to the analysis and evaluations, it aims to reveal the physical origin and formation of galaxies in different stages, as well as their physical relationships with large-scale structures, and then summarize the universal physical laws affecting galaxy formation. Moreover, the current limitations of the state-of-art results will be demonstrated and prospects will be given accordingly. Overall, these results shed light on guiding further exploration of investigation of star formation.